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NGC 4636 Background Subtracted
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NGC 4636:
Hot Galactic Arms Point To Vicious Cycle

NGC 4636
Credit: NASA/SAO/CXC/C.Jones et al.

Chandra's image of the elliptical NGC 4636 shows spectacular symmetric arms, or arcs, of hot gas extending 25,000 light years into a huge cloud of multimillion-degree-Celsius gas that envelopes the galaxy. At a temperature of 10 million degrees, the arms are 30 percent hotter than the surrounding gas cloud.

The temperature jump, together with the symmetry and scale of the arms indicate that the arms are the leading edge of a galaxy-sized shock wave that is racing outward from the center of the galaxy at 700 kilometers per second. An explosion with an energy equivalent to several hundred thousand supernovas would be required to produce this effect.

This eruption could be the latest episode in a feedback cycle of violence that keeps the galaxy in a state of turmoil. The cycle starts when a hot gas cloud that envelops the stars in the galaxy cools and falls inward toward a central, massive black hole. The feeding of the black hole by the infalling gas leads to an explosion that heats the hot gaseous envelope, which then cools over a period of several million years to begin the cycle anew.

Fast Facts for NGC 4636:
Credit  NASA/SAO/CXC/C.Jones et al.
Scale  Image is 5 x 4 arcmin across.
Category  Normal Galaxies & Starburst Galaxies
Coordinates (J2000)  RA 12h 42m 50s | Dec +02° 41' 17"
Constellation  Virgo
Observation Dates  January 26-27, 2000
Observation Time  15 hours
Obs. IDs  323
Color Code  Intensity
Instrument  ACIS
Distance Estimate  50 million light years
Release Date  December 19, 2001